Protoneutron star cooling with convection: The effect of the symmetry energy

Physical Review Letters

Volumn 108, Issue 6, 2012, Pages

  Roberts, L F ^a   Shen, G ^b   Cirigliano, V ^b   Pons, J A ^c   Reddy, S ^b,d   Woosley, S E ^a  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b LOS ALAMOS NATIONAL LABORATORY   (United States)

^c UNIVERSITY OF ALICANTE   (Spain)

^d UNIVERSITY OF WASHINGTON   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

BARYON DENSITY; CONVECTIVE INSTABILITIES; EQUATION OF STATE; NEUTRINO EMISSION; NEUTRON STARS; NUCLEAR DENSITIES; NUCLEAR SYMMETRY ENERGY; SPATIAL EXTENT; SUPERNOVA EXPLOSION; TIME-PERIODS;

ELEMENTARY PARTICLES; EQUATIONS OF STATE;

STARS;

EID: 84856812446     PISSN: 00319007     EISSN: 10797114     Source Type: Journal    
DOI: 10.1103/PhysRevLett.108.061103     Document Type: Article

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